Forbush decreases recorded by the URAGAN muon hodoscope in 2006-2011. Bulletin of the Russian Academy of Sciences: Physics Volume 77, Issue 5, May 2013, Pages 532-534
14 сентября 2018
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Вид публикации | Статья |
Контактные данные автора публикации | Barbashina, N.S. , Astapov, I.I., Borog, V.V., Dmitrieva, A.N., Kokoulin, R.P., Kompaniets, K.G., Mishutina, Yu.N., Petrukhin, A.A., SitKo, O.A., Shutenko, V.V., Yakovleva, E.I., Yashin, I.I. National Research Nuclear University MEPhI |
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Аннотация
Variations in the cosmic ray muon flux on Earths surface during Forbush decreases (FD) recorded by the URAGAN muon hodoscope in 2006-2011 are investigated. The dependence of the rate of amplitude reduction on the primary particle energy in a range above 10 GeV at different phases of FD development is studied by analyzing the variations in the cosmic ray muon flux recorded with the hodoscope. Analytical data on the spatial and angular dynamics of the muon flux are used to estimate variations in the spatial anisotropy of the muon flux during FDs. © 2013 Allerton Press, Inc.
Indexed keywords
Analytical data; Cosmic-ray muons; Earths surface; Forbush decrease; Muon flux; Muon hodoscopes; Primary particle energy; Spatial anisotropy
ПодробнееIndexed keywords
Analytical data; Cosmic-ray muons; Earths surface; Forbush decrease; Muon flux; Muon hodoscopes; Primary particle energy; Spatial anisotropy
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